Another proposal to understand the dark energy problem is to modify the gravitational Einstein-Hilbert action known as modified gravity theories, including \(f(R)\)  theory [1]}, [2]}, \(f(T)\)  theory [3]}, [4]}, \(f(R,T)\)  theory [5]}, [6]}. Theories of gravity can be classified into three categories based on their connection. They are as follows: the Levi-Civita connection and curvature; the metric tetrads and torsion; and the third employs a torsion and curvature free symmetric teleparallel connection that is not metric compatible. By requiring that the curvature vanishes, and the connection is torsionless, the remaining gravitational interaction is endowed by non-metricity \(Q\) . Here, \(Q\)  geometrically describes the variation of the length of a vector in the parallel transport. In the present article, we will work with the extension of the recently introduced \(f(Q)\)  theory of gravity [7]}, [8]}, known as \(f(Q,T)\)  gravity [9]}, where \(Q\)  is the non-metricity and \(T\)  is the trace of the energy-momentum tensor. Despite its newness, the \(f(Q,T)\)  theory has some intriguing and useful applications in the literature. The first cosmological implications in \(f(Q,T)\)  gravity appear in Reference [9]}, while late-time accelerated expansion with observational constraints can be seen in [11]}, [12]}. To get in touch with other works in \(f(Q,T)\)  theory, one can check references [13]}, [14]}, [15]}, [16]}.
